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- W3105432013 endingPage "1088" @default.
- W3105432013 startingPage "1066" @default.
- W3105432013 abstract "Archival Chandra observations are used to study the X-ray emission associated with star formation in the central region of the nearby SAB(s)cd galaxy NGC 2403. The distribution of X-ray emission is compared to the morphology visible at other wavelengths using complementary Spitzer, GALEX, and ground-based Halpha imagery. In general, the brightest extended X-ray emission is associated with HII regions and to other star-forming structures but is more pervasive; existing also in regions devoid of strong Halpha and UV emission. This X-ray emission has the spectral properties of diffuse hot gas (kT ~ 0.2keV) whose likely origin is in gas shock-heated by stellar winds and supernovae with < 20% coming from faint unresolved X-ray point sources. This hot gas may be slowly-cooling extra-planar remnants of past outflow events, or a disk component that either lingers after local star formation activity has ended or that has vented from active star-forming regions into a porous interstellar medium." @default.
- W3105432013 created "2020-11-23" @default.
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- W3105432013 date "2010-02-03" @default.
- W3105432013 modified "2023-09-25" @default.
- W3105432013 title "AN X-RAY VIEW OF STAR FORMATION IN THE CENTRAL 3 kpc OF NGC 2403" @default.
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- W3105432013 doi "https://doi.org/10.1088/0004-6256/139/3/1066" @default.
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